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IC/66/81
INTERNATIONAL ATOMIC ENERGY AGENCY
INTERNATIONAL CENTRE FOR THEORETICAL
PHYSICS
ON FACTORIZATIONOF EINSTEIN'S FORMALISM INTO A PAIR
OF QUATERNION FIELD EQUATIONS
M. SACHS
1966PIAZZA OBERDAN
TRIESTE
IC/66/S1
INTERNATIONAL ATOMIC ENERGY AGENCY
INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS
ON FACTORIZATION OF EINSTEIN'S FORMALISM
INTO A PAIR OF QUATERNION FIELD EQUATIONS *"*
M. SACHS**
TRIESTE
July 1966
' To be submitted to Nuovo Cirnento* The research reported in this paper has been sponsored by the Air Force Cambridge Research Laboratories, Office of
Aerospace Research, under Contract AF 19(628)-2816** On leave of absence from Dept. of Physics, Boston University, Boston, Mass., USA
Permanent address after September, 1966: Dept. of Physics, State University of New York, Buffalo, N.Y., USA
ABSTRACT
It is proposed that a full exploitation of the principle of general
relativity in the construction of the metrical field equations implies that
the fundamental variables should be quaternion fields rather than the
metric tensor field of the conventional formulation. Thus, the tensor
property of Einstein's formalism is replaced here by a formalism that
transforms as a quaternion - a vector field in co-ordinate space and a
second-rank spinor field of the type >? 383 >\ in spinor space. The geo-
metrical field variables of the Riemann space are derived in quaternion
form. The principle of least action ^vith the Palitini technique) is then used
to derive a pair of time-reversed quaternion field equations, from the
(quaternionic form of ) Einstein1 s Lagrangian, It is then shown how the
conventional tensor form of the Einstein formalism is recovered from a
particular combination of the derived time-reversed quaternion equations.
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ON FACTORIZATION OF EINSTEIN'S FORMALISM INTO A PAIR OF
QUATERNION FIELD EQUATIONS
1. INTRODUCTION
Shortly after Dirac1 s discovery of the special relativistic spinor
wave equation, several investigations were initiated to study the role of
spinor variables in a generally relativistic formalism. It was found that,
indeed, the Riemannian manifold could alternatively be described in terms
of four four-vector fields at each space-time point (i. e., a tetrad field)
rather than the usual metric tensor field.
In close connection with the latter formalism one may also con-
struct a theory of general relativity in which fundamental quaternion fields2
(and their conjugates) play the role of defining the metric field. Using the
c orres pondence
(1) <j°
or equivalently
(I1) ff f q f
where cr° is the unit two-dimensional matrix and "Tr" denotes the trace
the Einstein field equations
(2) R*u - i g ^ R = KT^
can be re-expressed in a form in which the quaternion variables fy ("*•> > ^
rather than g/1' X) are the field solutions of these equations. The quater-
nion variables have the structure
where vv^ are unit four-vectors with j/M' having a positive norm and hv/t*'
having negative norms. The conjugate quaternion to 0/ is its time-
reversed field, i .e . , the quaternionic basis elements for QM are (o"k* er°)
while those of q/ are (0" )"(T ) where or * are the usual three Pauli
matrices. This definition of quaternion conjugation is equivalent to the
following relationship:
(3)
where e - (_\ J
and the asterisk denotes complex conjugation. Finally, it is readily veri-
fied that with the normalization of ^V* defined above, an invariant of the
Riemannian manifold is
(4) q^ V s q^ q A = " 4
It is important to note that the quaternion fields transform in co-
ordinate space as four-vectors and that they have additional transformation
properties in an "internal space" - both the quaternion and its conjugate
behave in spinor space as a second-rank spinor of the type V) H i *".
An implication of the property of q/UV as a bilinear product in
< and "a. , is that the Einstein field equations (in o " ^ ) might factor
into two (time-reversed) equations which separately transform as quaternion
fields. The purpose of this paper is to demonstrate such a "factorization".
2. THE VARIABLES OF THE RIEMANN SPACE IN QUATERNION
FORM
It follows from the invariance of the metric Q^^v that the
covariant derivatives of the quaternion fields must vanish. The covariant
derivative, in turn, depends on two distinct parts - one that relates to a
change in spinor space and the other to a change in co-ordinate space.
Denoting the former degrees of freedom in terms of the spinor components
of the quaternion and the latter by [ P j , we have
(5)
where the cova riant derivative of a spinor field w defines the spin-affine
connection ^ i p as follows
(6) rj. p = (9j> +n_p)»7
It is readily verified that as a consequence of the vanishing of the covariant
derivatives of Q K , "W, has the two equivalent forms
(7) Q?* \ fyq* + r^pqT) q& = - ~ q * *
where | PT i is the ordinary affine connection.
Combining Eqs. (6) and (5), the following relationship follows
Since the last term on the right-hand side of Eq. (8) refers only to the behaviour
of the quaternion as a vector in co-ordinate space, it relates to the Riemann
curvature tensor , i. e.,
0) fV];f;*" [ V ] ^ ^ = R/"tj*<i*
With the definition (6) of spin-affine connection and denoting the spin curvature
by Kc,\ > we have
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Substituting Eqs. (9) and (10) into Eq. (8) frnd dropping the spinor component
indices) the following equation results
(Ha) (KfX q^ + qAK^x) = - R^HJ* q *
where the "dagger" denotes the hermitian adjoint. It is also readily veri-
fied from the vanishing of the covariant derivatives of the conjugate quater-
nion and the relationship (3) that the time-reversed equation which accom-
panies Eq. (lla) is
(lib) Kf* V1" VK i* ' R^^qK
Finally, if we multiply Eq. (lla) on the right with cj, and Eq. (lib)
on the left with <^K , add the resulting equations and make use of the follow-
ing identity (for K fixed)
the following expression for the Riemann curvature tensor results
(12) <?° RAHfA = | [Kj,* q , ^ - qK q^ Kfx + q^ K J A qK - q,
Taking the trace of both sides of Eq. (12) the coefficients of the curvature
tensor can then be expressed in the form
(12') RAKpA = ~ Tr iKpAiq^ qK - qK q J + h. c.
where "h. c. " denotes the hermitian conjugate matrix field.
The Ricci tensor may now be obtained in the usual way by con-
tracting tWKpX with the contravariant metric tensor
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RKf = \ [KpX q* qK - qK qA Kf\
(13)
The trace of this equation then gives the components of the Ricci tensor
(13') RKf =±Tr[Kj,*{q*qk - qK qX) + h. c. ]
Finally, the scalar curvature of the Riemann space is
R = gK?RKj) =^TrtKj?A(q'1 qP - qJ5 q*) + h . c ]
If we use the fact that
the scalar curvature then reduces to the form
(14) R = | Tr [q> K ^ q* + h. c. ]
To sum up, the respective expressions in a Riemann space for the
metric tensor, curvature tensor, Ricci tensor and scalar curvature, in
terms of the spinor-quaternion formalism, are given in Eqs. (1), (12), (13)
and (14).
3. DERIVATIONS OF THE METRICAL FIELD EQUATIONS FROM
THE PRINCIPLE OF LEAST ACTION
3Einstein's well-known derivation of the field Eq. (2) follows from
a minimization of the action functional
(15) A = A 6+AH
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where
(16) AG = f/gd* x = f R /^g d* x
and A^ is the contribution due to matter and electromagnetic fields. In
this variational procedure it is assumed that only the components of the
metric tensor q^ are the independent field variables and that all fields
are non-singular.
4There is also the alternative technique of Palitini for deriving
the field Eq. (2) from the minimization of oC which takes both the metric :
tensor Q, v and the components of the affine connection fl vf to be the in-
dependent variables. The latter technique gives two sets of field equations.
The first, in q^ , does not relate the metric tensor to the affine connect-
ion. , The second, in f \, , leads to the vanishing of the covariant de-
rivatives of the metric tensor field which, in turn, implies the mathematical
relation between P*, and derivatives of g^ . Thus the Palitini technique
gives field equations that are equivalent to Einstein's equations; yet it treats
the coefficients (P v 1 in a more general way thereby allowing the pos-
sibility of extending the theory by generalizing the affine connection.
In the derivation that follows, the Palitini technique will be
utilized to derive the quaternionic form of the metrical field equations. The
Lagrangian will be taken, in the variational calculation, as a function of the
independent variables
and their conjugates, where the following notation is used :
(17) ^Wf a (8J>+ «/) *K»
The spin curvature in Eq. (10) is then expressible in the form
(18)
If # and B are any two matrix fields, it follows that
a 9 t- Tr(AB) = Aii or -5-5 T^AB).55 A1
j J 9B
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AAV
Using the correspondence (1) between q and the quaternion variables,
the derivatives of the metric density with respect to the latter fields are as
follows
r ("4 T r
(20)
With the relationship (19) in Eq. (20) and the hermitian property of the
quaternions it follows that
Finally, with the relationship (14) in the Lagrangian
using Eq. (21) and the anti- symmetric property of the spin curvature
it follows that
(22a) f | ? = [ | (qA KTpA + KpX q>) + | R q f]* sf- g
In a similar fashion, the following accompanying time-reversed relation is
obtained:
(22b) f e = [ - \ (KTp qA + q* KfK) + I R ^ ] * / - g
Since dCG does not have any explicit dependence on derivatives
of the quaternion fields, the substitution of Eqs. (22) into the Lagrange-
Euler formalism yields the following field equations;
(23a) 7 (KpX q* + qX KJJ ) + £ R qp = K TP(K^ q + q Kjj ) + | R qf
(23b) - | (KJA qX + q Kf*) + | R q = K(rO) )
where 0 , is the (complex conjugate of the) vector field which is obtained
from a minimization (with respect to the quaternion variables) of the rest
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of the Lagrangian that depends on the matter variabLes. The right-hand
side of Eq. (23b)
is the time-reversal of the source field X in Eq. (23a).
Finally, we shall shall determine the relationship between the
spin-affine connection oi^ and the quaternion fields from the independent
variation of oT with respect to Sl^ and *>l<L\ ^ . Since X^ depends
on the affine connection through the spin curvature K e which in turn
depends only on ti^-p, and not <>>l« itself (Eq. (18), the variational procedure
applied to these fields gives the following result:
&.L - «rWith Q r and a r arbitraryj the preceding equation implies that the covariant
derivatives of the quaternion fields themselves must be zero. This result, in
turn, leads to the relationship (7) between the spin-affine connection and the
derivatives of the fundamental quaternion fields. The combination of thefield equations (23) together with the restrictions (7) on the spin-affine
connection then constitutes the quaternionic form for the differential relation
ships for the metric field of a Riemannian space.
While the explicit structure of TL in the field Eqs. (23) is an
important aim of the present programme of study, the main object of this
paper has been to show that the second-rank tensor form (2) of Einstein's
field equations does indeed decompose into two separate quaternion field
equations. These transform in co-ordinate space like vector field equations
while they behave like second-rank spinors of the type if] S ''j under trans-
formations in spinor space. The separate field Eqs. (23a) and (23b) are,
in fact, the time-reversals of each other. Thus, the "factorization" (23) of
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Einstein's Eqs, (2) is somewhat analogous to the factorization of the Klein-
Gordon equation
_ o . . fa*, 9 v? = -mX
into the two time-reversed two-component Dirac spinor equations in >\
and "V , The spinor form of Dirac1 s equation is, of course, more general
than the Klein-Gordon equation because 1) it entails extra degrees of
freedom in the spinor variables and 2) it allows non-reflection symmetric
interactions to appear - terms that would have no counterpart in a scalar
formalism. The quaternion forms (23) of the metrical field equations are
more general than the tensor form of Einstein's field equations for precisely
the same reasons. Since the postulate of relativity theory does not have to
do with reflection symmetry at all, it is contended that the quaternion form
(23) of the metrical field equations represents a full exploitation of the
principle of relativity in the construction of the field equations.that describe
gravitational forces.
4. A RECOVERY OF THE TENSOR FORM OF EINSTEIN'S
EQUATIONS
As a final step in this analysis it will be shown that a particular
combination of the time-reversed Eqs. (23a) and (23b) does indeed give back
the usual tensor form of Einstein's equations.
If we multiply Eq. (23a) on the right with^ and Eq. (23b) on the
left with Q.T and add the resulting equations, the following relation is
obtained:
\
(25)
qy (rTf)]y (rTf)
Thus, with the definitions (13) and (1) for the Ricci tensor and metric tensor,
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Kq. (25) takes the Einstein form
where
is the "matter source" of the metrical field in the tensor form of these
equations.
5. CONCLUDING REMARKS
Summarizing, we have seen that the second-rank tensor form of
the Einstein field equations decomposes into a pair of quaternion equations
that are related to each other by time reversal. Thus the complexity of
the second-rank tensor field is reduced to a pair of vector fields while the
spinor degrees of freedom which were absent ("masked") in the single
tensor equations appear in the separated quaternion equations. The root
of this result lies, in fact, in the properties of the irreducible represent-
ations of the subgroup of rotations of the Einstein group. The lowest
dimensional .representations of this group in fact behave as second-rank
spinors of the quaternionic type ft JS Kl * . The latter represent a group
in which reflection symmetry elements are not defined while the larger
dimensional representations which underlie the Einstein1 s original tensor
formulation do admit reflection symmetry in space and time into the group.
Since the principle of relativity deals only with continuous trans-
formations in space and time, the quaternionic representations (which are
the lowest dimensional representations) then relate to the most general
expression of the theory. Indeed, within the formalism presented here,
we have seen that the usual form of Einstein's equations results only from
one particular way of combining the quaternion field Eq. (23a) with its time-
reversed Eq. (23b). It can then be conjectured that the separate use of
these equations should yield results that are out of the realm of prediction
of the tensor equations.
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Finally, it might be remarked that the quaternion form of the
metrical field equations lends itself in a natural way to a unification between
the inertial and gravitational manifestations of interacting matter. This is
because of the basic expression of the matter fields themselves in terms7
of the same spinor and quaternion variables. Studies of the possibility
of unification along these lines are currently in progress.
ACKNOWLEDGMENTS
I would like to thank Professor Abdus Salam and the IAEA for
hospitality at the International Centre for Theoretical Physics, Trieste,
during the summer, 1966, when this work was completed.
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REFERENCES AND FOOTNOTES
1. A. EINSTEIN, Math. Ann. 102, 685 (1930);
H. S. RUSE, Prac . Roy. Soc. (Edinburgh) j[7, 97(1937).
2. For an application of the quaternion formalism in general relativity toelectromagnetic theory, see
M. SACHS, Nuovo Cimento jU, 98 (1964). A recent survey of work
on the spinor formalism in a Riemannian space is given by CAP,
MAJEROTTO, RAAB and UNTEREGGER, Fortsch. d. Phys. l±, 205
(1966).
3. See, for example, ADLER, BAZIN and SCHIFFER, Introduction to
General Relativity (McGraw Hill Book Co., New York, 1965).
4. See E. SCHRODINGER, Space-Time-Matter (Cambridge University
Press, 1963) Chap. XII.
5. Note that the spin-affine connection-Q^ transforms covariantly as a
vector in co-ordinate space while it does not, by itself, transform
covariantly in spinor space. It is rather the combination ^'jfyu.+-£\/u?)rl
that behaves as a scalar in spinor space (as well as co-ordinate space).
This, of course, is analogous to the non-covariance of C , by itself
in co-ordinate space. Using the Palitini technique, the independent
variables .0 ,1^ in the variational procedure are continuous fields, but
they are not by themselves covariant entities. They are only used in
the mathematical procedure of the variational method to derive the
field equations.
6. Note that the field equations in the spin-affine connection will be some-
what altered from Eq. (24) when the generally covariant form of the
matter fields are included in the Lagrangian formalism. This is
because of the dependence of the latter differential forms on M u, .
The effect of this addition would then be to alter the relationship (7)
in such a way as to add the contribution from the spinor formalism of
the matter fields themselves.
7. M. SACHS, Nuovo Cimento 34, 81 (1964).
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